Abstract
The relationship between the cosmic ray intensity and solar activity during solar cycle 20 is discussed. A model is developed whereby it is possible to simulate the observed cosmic ray intensity from the observed number of solar flares of importance ⩾1. This model leads to a radius for the modulation region of 60–70 AU. It is suggested that high speed solar streams also made a small contribution to the modulation of cosmic rays during solar cycle 20.
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Hatton, C.J. Solar flares and the cosmic ray intensity. Sol Phys 66, 159–165 (1980). https://doi.org/10.1007/BF00150526
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DOI: https://doi.org/10.1007/BF00150526